Image Details
Caption: Figure 10.
Selected line profile fits for the ET Cru primary component from FEROS spectra. Observed spectra are shown as black dots, with the best-fit synthetic spectra overlaid in red. The dashed horizontal line indicates the continuum level. The derived logarithmic abundance (logϵ) for each species is indicated in the corresponding panel.
© 2026. The Author(s). Published by the American Astronomical Society.